Zoom Forward 08 Colorful Universe

If you do not “Zoom Forward” in your Spiritual Life and prepare for your departure from this Earth Life, then you have made a very grievous mistake. There is more to your Life than the people and things of this Earth Life…
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Regardless of who you are; or who you think you are and likewise concerning what you have or what you think you have and you can place any name or anything in the equation: If you are not extremely careful; you will spend your entire life focused on the people and things surrounding you and they will absorb, deceive and trick you so much, you will miss out towards seeking the Lord.
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Your life on earth is only a “limited amount of time”; then you pass away into the eternal state, into infinity, through the:  Gate of Eternity  for better or worse!!!
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Be wise and seek the Lord while you have “time”.
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You need to buy up, that is, make better use of the “time in your life” as to being rich toward God with whatever “time you have”; because there is a limited amount of the “time in your life” and you cannot buy/get it back, once it is gone!!!
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There will be a “time in your life” that your soul will be required of you; and you are powerless to stop it from leaving your earth body.
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Luke 12: [13] And one of the company said unto him, Master, speak to my brother, that he divide the inheritance with me. [14] And he said unto him, Man, who made me a judge or a divider over you? [15] And he said unto them, Take heed, and beware of covetousness: for a man’s life consisteth not in the abundance of the things which he possesseth. [16] And he spoke a parable unto them, saying, The ground of a certain rich man brought forth plentifully: [17] And he thought within himself, saying, What shall I do, because I have no room where to bestow my fruits? [18] And he said, This will I do: I will pull down my barns, and build greater; and there will I bestow all my fruits and my goods. [19] And I will say to my soul, Soul, thou hast much goods laid up for many years; take thine ease, eat, drink, and be merry. [20] But God said unto him, Thou fool, this night thy soul shall be required of thee: then whose shall those things be, which thou hast provided? [21] So is he that layeth up treasure for himself, and is not rich toward God.
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The following are about the Universe. There is a life beyond Earth. As people upon this Earth; the great majority of humanity has been deceived by people and things; as if this is all of our existence. Perhaps this page will be helpful to someone; towards helping you to awaken to the reality of Life after this Earth Life…
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https://www.nasa.gov/nasa-brand-center/images-and-media/

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From:  https://science.nasa.gov

As of December 2023, there are at least 200 articles I plan to add and probably many more, as they are created at NASA; to this website; well, maybe… I enjoyed viewing and reading the articles, so perhaps they will be of interest to anyone viewing this website.

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Colorful Universe

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NASA’s James Webb Space Telescope and Hubble Space Telescope have united to study an expansive galaxy cluster known as MACS0416. The resulting panchromatic image combines visible and infrared light to assemble one of the most comprehensive views of the universe ever taken. Located about 4.3 billion light-years from Earth, MACS0416 is a pair of colliding galaxy clusters that will eventually combine to form an even bigger cluster.

Image: Galaxy Cluster MACS0416

This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from NASA’s James Webb Space Telescope with visible-light data from NASA’s Hubble Space Telescope. The resulting wavelength coverage, from 0.4 to 5 microns, reveals a vivid landscape of galaxies whose colors give clues to galaxy distances: The bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant, or else contain copious amount of dust, as detected by Webb. The image reveals a wealth of details that are only possible to capture by combining the power of both space telescopes. In this image, blue represents data at wavelengths of 0.435 and 0.606 microns (Hubble filters F435W and F606W); cyan is 0.814, 0.9, and 1.05 microns (Hubble filters F814W, and F105W and Webb filter F090W); green is 1.15, 1.25, 1.4, 1.5, and 1.6 microns (Hubble filters F125W, F140W, and F160W, and Webb filters F115W and F150W); yellow is 2.00 and 2.77 microns (Webb filters F200W, and F277W); orange is 3.56 microns (Webb filter F356W); and red represents data at 4.1 and 4.44 microns (Webb filters F410M and F444W).
NASA, ESA, CSA, STScI, J. Diego (Instituto de Física de Cantabria, Spain), J. D’Silva (U. Western Australia), A. Koekemoer (STScI), J. Summers & R. Windhorst (ASU), and H. Yan (U. Missouri).

The image reveals a wealth of details that are only possible to capture by combining the power of both space telescopes. It includes a bounty of galaxies outside the cluster and a sprinkling of sources that vary over time, likely due to gravitational lensing – the distortion and amplification of light from distant background sources.

This cluster was the first of a set of unprecedented, super-deep views of the universe from an ambitious, collaborative Hubble program called the Frontier Fields, inaugurated in 2014. Hubble pioneered the search for some of the intrinsically faintest and youngest galaxies ever detected. Webb’s infrared view significantly bolsters this deep look by going even farther into the early universe with its infrared vision.

“We are building on Hubble’s legacy by pushing to greater distances and fainter objects,” said Rogier Windhorst of Arizona State University, principal investigator of the PEARLS program (Prime Extragalactic Areas for Reionization and Lensing Science), which took the Webb observations.

What the Colors Mean

To make the image, in general the shortest wavelengths of light were color-coded blue, the longest wavelengths red, and intermediate wavelengths green. The broad range of wavelengths, from 0.4 to 5 microns, yields a particularly vivid landscape of galaxies.

Those colors give clues to galaxy distances: The bluest galaxies are relatively nearby and often show intense star formation, as best detected by Hubble, while the redder galaxies tend to be more distant as detected by Webb. Some galaxies also appear very red because they contain copious amounts of cosmic dust that tends to absorb bluer colors of starlight.

“The whole picture doesn’t become clear until you combine Webb data with Hubble data,” said Windhorst.

Image: Side-by-side Hubble/Webb

This side-by-side comparison of galaxy cluster MACS0416 as seen by the Hubble Space Telescope in optical light (left) and the James Webb Space Telescope in infrared light (right) reveals different details. Both images feature hundreds of galaxies, however the Webb image shows galaxies that are invisible or only barely visible in the Hubble image. This is because Webb’s infrared vision can detect galaxies too distant or dusty for Hubble to see. (Light from distant galaxies is redshifted due to the expansion of the universe.) The total exposure time for Webb was about 22 hours, compared to 122 hours of exposure time for the Hubble image.
NASA, ESA, CSA, STScI

Christmas Tree Galaxy Cluster

While the new Webb observations contribute to this aesthetic view, they were taken for a specific scientific purpose. The research team combined their three epochs of observations, each taken weeks apart, with a fourth epoch from the CANUCS (CAnadian NIRISS Unbiased Cluster Survey) research team. The goal was to search for objects varying in observed brightness over time, known as transients.

They identified 14 such transients across the field of view. Twelve of those transients were located in three galaxies that are highly magnified by gravitational lensing, and are likely to be individual stars or multiple-star systems that are briefly very highly magnified. The remaining two transients are within more moderately magnified background galaxies and are likely to be supernovae.

“We’re calling MACS0416 the Christmas Tree Galaxy Cluster, both because it’s so colorful and because of these flickering lights we find within it. We can see transients everywhere,” said Haojing Yan of the University of Missouri in Columbia, lead author of one paper describing the scientific results.

Finding so many transients with observations spanning a relatively short time frame suggests that astronomers could find many additional transients in this cluster and others like it through regular monitoring with Webb.

A Kaiju Star

Among the transients the team identified, one stood out in particular. Located in a galaxy that existed about 3 billion years after the big bang, it is magnified by a factor of at least 4,000. The team nicknamed the star system “Mothra” in a nod to its “monster nature,” being both extremely bright and extremely magnified. It joins another lensed star the researchers previously identified that they nicknamed “Godzilla.” (Both Godzilla and Mothra are giant monsters known as kaiju in Japanese cinema.)

Interestingly, Mothra is also visible in the Hubble observations that were taken nine years previously. This is unusual, because a very specific alignment between the foreground galaxy cluster and the background star is needed to magnify a star so greatly. The mutual motions of the star and the cluster should have eventually eliminated that alignment.

Image: Gravitationally Lensed Galaxy

This image of galaxy cluster MACS0416 highlights one particular gravitationally lensed background galaxy, which existed about 3 billion years after the big bang. That galaxy contains a transient, or object that varies in observed brightness over time, that the science team nicknamed “Mothra.” Mothra is a star that is magnified by a factor of at least 4,000 times. The team believes that Mothra is magnified not only by the gravity of galaxy cluster MACS0416, but also by an object known as a “milli-lens” that likely weighs about as much as a globular star cluster.
NASA, ESA, CSA, STScI, J. Diego (Instituto de Física de Cantabria, Spain), J. D’Silva (U. Western Australia), A. Koekemoer (STScI), J. Summers & R. Windhorst (ASU), and H. Yan (U. Missouri).

The most likely explanation is that there is an additional object within the foreground cluster that is adding more magnification. The team was able to constrain its mass to be between 10,000 and 1 million times the mass of our Sun. The exact nature of this so-called “milli-lens,” however, remains unknown.

“The most likely explanation is a globular star cluster that’s too faint for Webb to see directly,” stated Jose Diego of the Instituto de Física de Cantabria in Spain, lead author of the paper detailing the finding. “But we don’t know the true nature of this additional lens yet.”

The Yan et al. paper is accepted for publication in The Astrophysical Journal. The Diego et al. paper has been published in Astronomy & Astrophysics.

The Webb data shown here was obtained as part of PEARLS GTO program 1176.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble and Webb science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, in Washington, D.C.

Media Contacts

Laura Betzlaura.e.betz@nasa.gov, Claire Andreoliclaire.andreoli@nasa.gov
NASA’s  Goddard Space Flight Center, Greenbelt, Md.

Hannah Braun hbraun@stsci.edu , Christine Pulliamcpulliam@stsci.edi
Space Telescope Science Institute, Baltimore, Md.